Cosmology with the eROSITA all-sky survey of galaxy clusters
Cosmology with the eROSITA all-sky survey of galaxy clusters
Cosmology with the eROSITA all-sky survey of galaxy clusters
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SKA (and pathfdrs) & <strong>galaxy</strong> <strong>clusters</strong>• Radio-‐halo detected <strong>clusters</strong> vs. X-ray detected <strong>clusters</strong> • Dynamical state classificaFon and X-ray scaling relaFons (e.g. H.Roefgering’s talk) • AGN past acFvity (radio bubbles, etc.) è Feedback in <strong>the</strong> ICM • Relics (past merging acFvity, shocks) • Non-‐<strong>the</strong>rmal X-‐ray emission quanFfiable (CRS=Central Radio Source) Mifal+11 Wing&Blanton 11 • Bended radio tails (distant <strong>clusters</strong> searches) [e.g. Blanton+03] • Cross-‐correlaFons radio-‐gal/X-‐ray (extended/point-‐sources/background) Van Weeren et al. N. Clerc – Oxford – 17 Sept. 2013
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